全文获取类型
收费全文 | 10052篇 |
免费 | 1775篇 |
国内免费 | 1597篇 |
专业分类
航空 | 7195篇 |
航天技术 | 2557篇 |
综合类 | 1244篇 |
航天 | 2428篇 |
出版年
2024年 | 71篇 |
2023年 | 230篇 |
2022年 | 321篇 |
2021年 | 472篇 |
2020年 | 501篇 |
2019年 | 629篇 |
2018年 | 723篇 |
2017年 | 611篇 |
2016年 | 622篇 |
2015年 | 549篇 |
2014年 | 646篇 |
2013年 | 547篇 |
2012年 | 704篇 |
2011年 | 829篇 |
2010年 | 581篇 |
2009年 | 509篇 |
2008年 | 646篇 |
2007年 | 623篇 |
2006年 | 599篇 |
2005年 | 475篇 |
2004年 | 416篇 |
2003年 | 307篇 |
2002年 | 226篇 |
2001年 | 227篇 |
2000年 | 167篇 |
1999年 | 161篇 |
1998年 | 171篇 |
1997年 | 129篇 |
1996年 | 112篇 |
1995年 | 104篇 |
1994年 | 122篇 |
1993年 | 75篇 |
1992年 | 71篇 |
1991年 | 61篇 |
1990年 | 66篇 |
1989年 | 60篇 |
1988年 | 39篇 |
1987年 | 14篇 |
1986年 | 3篇 |
1984年 | 4篇 |
1981年 | 1篇 |
排序方式: 共有10000条查询结果,搜索用时 78 毫秒
201.
董富祥 《中国空间科学技术》2020,40(3):76-82
为识别二维二次太阳翼关键环节和预示其在轨展开故障模式,开展不同位置绳索断裂失效对太阳翼展开的影响程度分析。采用考虑绳索断裂的绳索联动轮力学模型,建立了适应于不同联动轮半径的联动轮受力模型,提出角度触发约束消除方法,解决了太阳翼第2次展开过程连续仿真问题,建立了太阳翼第2次展开动力学方程,分析了不同位置绳索断裂失效对太阳翼各板展开角度、展开构型和其他绳索张力的影响。分析表明,越靠近星体的绳索联动机构失效对太阳翼展开过程的影响越大,其中连接架上绳索联动机构失效可直接导致二维二次太阳翼在轨展开失败。 相似文献
202.
为了研究自由基型液体端羟基聚丁二烯预聚物(HTPB)体系官能度分布情况,对其化学合成中自由电子转移情况进行了分析,并通过数学统计的方法对其官能度分布进行理论数值模拟,建立了适用于自由基型HTPB官能度分布的函数关系式,并与GPC所测结果进行对比。结果显示,计算所得函数关系式与测试数据吻合结果较好,数值模拟结果准确性较高;自由基聚合生产的不同批次的HTPB官能度分布存在较大差异,单官能度分子含量可从5%~24%,二官能度分子的含量可从50%~81%;利用数学统计得到的函数关系,可将复杂的HTPB官能度测试转变为简单的分子量分布测试。 相似文献
203.
在深航近年来使用的承修商管理模式的基础上,通过实践不断修正,新增可视化质量评估平台,使深航的承修商管理形成一个完整的闭环监控,本文对这一可视化质量评估模型进行了详细介绍,以期为业内航材承修商管理工作提供参考。 相似文献
204.
王新 《长沙航空职业技术学院学报》2011,11(4):72-77
摘 运用文献资料法、专家访谈法、问卷调查法、数理统计法来进行调查与研究,从长沙市全民健身运动开展的体育资源利用实际情况出发,对长沙市全民健身运动开展的情况进行分析,根据全民健身运动过程中体育资源利用的情况,结合实际,提出了全民健身运动开展体育资源开发的对策,希望能为建立符合长沙市实际情况需要的全民健身运动发展模式寻求理... 相似文献
205.
航空测距器DME的开发、调试和性能验证都要用到高斯双脉冲调制格式的DME信号。由于专用的DME信号模拟器技术复杂、价格昂贵,人们常用具有快沿双脉冲调制功能的模拟信号源替代。本文以航空测距器DME信号要求为依据,初步分析了这种替代可能存在的问题,并通过实验对不同边沿条件下高斯双脉冲、矩形双脉冲调制信号的功率频谱占用情况进行了验证。 相似文献
206.
Paul A. Crowther Joanne L. Bibby James P. Furness J. Simon Clark 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
We highlight how the downward revision in the distance to the star cluster associated with SGR 1806–20 by Bibby et al. (2008) reconciles the apparent low contamination of BATSE short GRBs by intense flares from extragalactic magnetars without recourse to modifying the frequency of one such flare per 30 years per Milky Way galaxy. We also discuss the variety in progenitor initial masses of magnetars based upon cluster ages, ranging from ∼50 M⊙ for SGR 1806–20 and AXP CXOU J164710.2–455216 in Westerlund 1 to ∼17 M⊙ for SGR 1900+14 according to Davies et al. (2009) and presumably also 1E 1841–045 if it originated from one of the massive RSG clusters #2 or #3. 相似文献
207.
208.
《中国航空学报》2016,(3):746-753
X-ray pulsar-based navigation (XPNAV) is an attractive method for autonomous deep-space navigation in the future. The pulse phase estimation is a key task in XPNAV and its accuracy directly determines the navigation accuracy. State-of-the-art pulse phase estimation techniques either suffer from poor estimation accuracy, or involve the maximization of generally non-convex object function, thus resulting in a large computational cost. In this paper, a fast pulse phase estimation method based on epoch folding is presented. The statistical properties of the observed profile obtained through epoch folding are developed. Based on this, we recognize the joint prob-ability distribution of the observed profile as the likelihood function and utilize a fast Fourier transform-based procedure to estimate the pulse phase. Computational complexity of the proposed estimator is analyzed as well. Experimental results show that the proposed estimator significantly outperforms the currently used cross-correlation (CC) and nonlinear least squares (NLS) estima-tors, while significantly reduces the computational complexity compared with NLS and maximum likelihood (ML) estimators. 相似文献
209.
Chi-Ming Lee Chung-Yen Kuo Jian Sun Tzu-Pang Tseng Kwo-Hwa Chen Wen-Hau Lan C.K. Shum Tarig Ali Kuo-En Ching Philip Chu Yuanyuan Jia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(3):1280-1288
Global sea level rise due to an increasingly warmer climate has begun to induce hazards, adversely affecting the lives and properties of people residing in low-lying coastal regions and islands. Therefore, it is important to monitor and understand variations in coastal sea level covering offshore regions. Signal-to-noise ratio (SNR) data of Global Navigation Satellite System (GNSS) have been successfully used to robustly derive sea level heights (SLHs). In Taiwan, there are a number of continuously operating GNSS stations, not originally installed for sea level monitoring. They were established in harbors or near coastal regions for monitoring land motion. This study utilizes existing SNR data from three GNSS stations (Kaohsiung, Suao, and TaiCOAST) in Taiwan to compute SLHs with two methods, namely, Lomb–Scargle Periodogram (LSP)-only, and LSP aided with tidal harmonic analysis developed in this study. The results of both methods are compared with co-located or nearby tide gauge records. Due to the poor quality of SNR data, the worst accuracy of SLHs derived from traditional LSP-only method exceeds 1?m at the TaiCOAST station. With our procedure, the standard deviations (STDs) of difference between GNSS-derived SLHs and tide gauge records in Kaohsiung and Suao stations decreased to 10?cm and the results show excellent agreement with tide gauge derived relative sea level records, with STD of differences of 7?cm and correlation coefficient of 0.96. In addition, the absolute GNSS-R sea level trend in Kaohsiung during 2006–2011 agrees well with that derived from satellite altimetry. We conclude that the coastal GNSS stations in Taiwan have the potential of monitoring absolute coastal sea level change accurately when our proposed methodology is used. 相似文献
210.
Paul O’Brien 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The ASTROSAT satellite is an Indian National Space Observatory under development in India. Due for launch in 2010, ASTROSAT will carry a complement of five scientific instruments enabling simultaneous observations from the optical through to the hard X-ray energy band. This capability will enable broad-band spectroscopy and high time-resolution monitoring of both galactic and extra-galactic targets, such as X-ray binaries and AGN. One of the instruments is being built in collaboration with the Canadian Space Agency and another in collaboration with the University of Leicester. ASTROSAT also carries a scanning sky monitor to observe the variable X-ray sky. After an initial period of science verification and guaranteed time, a certain fraction of ASTROSAT observing time will also be made available to the community via a call for proposals. Here I summarise the instrument complement and principle scientific objectives of the mission. 相似文献